During Close Pass, Solar Orbiter Captures Venus' Glare 12 August 2021, by Miles Hatfield

Total Page：16

File Type：pdf, Size：1020Kb

During close pass, Solar Orbiter captures Venus' glare 12 August 2021, by Miles Hatfield planet. The rightmost is Omicron Tauri, and above and to the left of it is Xi Tauri, which is actually a quadruple star system. Both are part of the Taurus constellation. This was Solar Orbiter's second Venus flyby, with an Earth flyby in November 2021 and six more Venus flybys planned from 2022 to 2030. The spacecraft uses Venus' gravity to draw it closer to the Sun and tilt its orbit, swinging it up and out so as to "look down" on the Sun. From this vantage point, Solar Orbiter will eventually capture the first images of the Sun's north and south poles. Credit: NASA's Goddard Space Flight Center On Aug. 10, just one day later, ESA and the Japan Aerospace Exploration Agency's BepiColombo mission also flew by Venus. Learn more about the On Aug. 9, 2021, ESA/NASA's Solar Orbiter double flyby and see BepiColombo's images in spacecraft passed within 4,967 miles (7,995 ESA's coverage of the event. kilometers) of the surface of planet Venus. In the days leading up to the approach, the Solar Orbiter Heliospheric Imager, or SoloHI, telescope captured Provided by NASA's Goddard Space Flight Center this gleaming view of the planet. The images show Venus approaching from the left while the Sun is off camera to the upper right. The planet's nightside, the part hidden from the Sun, appears as a dark semicircle surrounded by a bright crescent of light – glare from Venus' incredibly bright sunlit side. "Ideally, we would have been able to resolve some features on the nightside of the planet, but there was just too much signal from the dayside." said Phillip Hess, astrophysicist at the Naval Research Laboratory in Washington, D.C. "Only a sliver of the dayside appears in the images, but it reflects enough sunlight to cause the bright crescent and the diffracted rays that seem to come from the surface." Two bright stars are also visible in the background early in the sequence, before being eclipsed by the 1 / 2 APA citation: During close pass, Solar Orbiter captures Venus' glare (2021, August 12) retrieved 27 September 2021 from https://phys.org/news/2021-08-solar-orbiter-captures-venus-glare.html This document is subject to copyright. Apart from any fair dealing for the purpose of private study or research, no part may be reproduced without the written permission. The content is provided for information purposes only. 2 / 2 Powered by TCPDF (www.tcpdf.org).

Copy Link

Recommended publications

Explore the Universe Observing Certificate Second Edition
RASC Observing Committee Explore the Universe Observing Certificate Second Edition Explore the Universe Observing Certificate Welcome to the Explore the Universe Observing Certificate Program. This program is designed to provide the observer with a well-rounded introduction to the night sky visible from North America. Using this observing program is an excellent way to gain knowledge and experience in astronomy. Experienced observers find that a planned observing session results in a more satisfying and interesting experience. This program will help introduce you to amateur astronomy and prepare you for other more challenging certificate programs such as the Messier and Finest NGC. The program covers the full range of astronomical objects. Here is a summary: Observing Objective Requirement Available Constellations and Bright Stars 12 24 The Moon 16 32 Solar System 5 10 Deep Sky Objects 12 24 Double Stars 10 20 Total 55 110 In each category a choice of objects is provided so that you can begin the certificate at any time of the year. In order to receive your certificate you need to observe a total of 55 of the 110 objects available. Here is a summary of some of the abbreviations used in this program Instrument V – Visual (unaided eye) B – Binocular T – Telescope V/B - Visual/Binocular B/T - Binocular/Telescope Season Season when the object can be best seen in the evening sky between dusk. and midnight. Objects may also be seen in other seasons. Description Brief description of the target object, its common name and other details. Cons Constellation where object can be found (if applicable) BOG Ref Refers to corresponding references in the RASC’s The Beginner’s Observing Guide highlighting this object.
[Show full text]
Adrian Zielonka's December Space and Astronomy News
Adrian Zielonka’s Astronomy and Space News Night Sky 2018 - December Sunrise Sunset Mercury Rises Venus Rises st st st st 1 – 7:52am 1 – 4:07pm 1 – 6:59am 1 – 4:10am th th th th 10 – 8:03am 10 – 4:04pm 10 – 6:10am 10 – 4:02am th th th th 20 – 8:11am 20 – 4:06pm 20 – 6:26am 20 – 4:03am th th th th 30 – 8:15am 30 – 4:13pm 30 – 7:03am 30 – 4:13am Moon Rise Moon Set Moon Rise Moon Set st st th th 1 – 12:34am 1 – 1:55pm 16 – 1:12pm 17 – 1:24am nd nd th th 2 – 1:50am 2 – 2:18pm 17 – 1:32pm 18 – 2:34am rd rd th th 3 – 3:04am 3 – 2:40pm 18 – 1:54pm 19 – 3:47am th th th th 4 – 4:18am 4 – 3:04pm 19 – 2:19pm 20 – 5:02am th th th st 5 – 5:30am 5 – 3:30pm 20 – 2:48pm 21 – 6:18am th th st nd 6 – 6:41am 6 – 4:00pm 21 – 3:26pm 22 – 7:33am (Full) th th nd rd 7 – 7:48am (New) 7 – 4:35pm (New) 22 – 4:13pm (Full) 23 – 8:42am th th rd th 8 – 8:49am 8 – 5:17pm 23 – 5:12pm 24 – 9:41am th th th th 9 – 9:44am 9 – 6:06pm 24 – 6:23pm 25 – 10:28am th th th th 10 – 10:30am 10 – 7:00pm 25 – 7:41pm 26 – 11:05am th th th th 11 – 11:08am 11 – 8:00pm 26 – 9:01pm 27 – 11:36am th th th th 12 – 11:40am 12 – 9:02pm 27 – 10:21pm 28 – 12:02pm th th th th 13 – 12:07pm 13 – 10:06pm 28 – 11:39pm 29 – 12:25pm (LQ) th th th th 14 – 12:30pm 14 – 11:11pm 30 – 12:54am 30 – 12:47pm th th st st 15 – 12:52pm (FQ) 16 – 12:17am 31 – 2:08am 31 – 1:10pm A useful site: www.heavens- above.com A S Zielonka There is a planned launch this month of a Chinese Long March 2D rocket from Jiuquan Satellite Launch Center, China.
[Show full text]
Annual Report 2011
Research Institute Leiden Observatory (Onderzoekinstituut Sterrewacht Leiden) Annual Report 2011 Sterrewacht Leiden Faculty of Mathematics and Natural Sciences Leiden University Niels Bohrweg 2 Postbus 9513 2333 CA Leiden 2300 RA Leiden The Netherlands http://www.strw.leidenuniv.nl Cover: Galaxy clusters grow by mergers with other clusters and galaxy groups. These mergers create shock waves within the intracluster medium (ICM) that can accelerate particles to extreme energies. In the presence of magnetic fields, relativistic electrons form large regions emitting synchrotron radiation, the so- called radio relics. A prime example of these phenomena can be found in the galaxy cluster 1RXS J0603.3+4214 (z = 0.225), recently discovered comparing radio and X-ray large sky surveys. The deep radio image on the front cover taken with the Giant Metrewave Radio Telescope (India) shows that this cluster hosts a spectacularly large bright 1.9 Mpc radio relic (Courtesy: van Weeren and Röttgering, et al.). Initial numerical simulations (Brüggen, van Weeren, Röttgering) indicate that the 1.9 Mpc shock can be explained as originating from a triple cluster merging. Studying such systems yield information on the physics of magnetic fields and particle acceleration as well properties of gas in merging clusters. An electronic version of this annual report is available on the web at http://www.strw.leidenuniv.nl/research/annualreport.php Production Annual Report 2011: A. van der Tang, E. Gerstel, A.S. Abdullah, H.E. Andrews Mancilla, F.P. Israel, M. Kazandjian, E. Deul Sterrewacht Leiden Executive (Directie Onderzoeksinstituut) Director K. Kuijken Wetenschappelijk Directeur Director of Education P. v.d.Werf Onderwijs Directeur Institute Manager E.
[Show full text]
Ephemerides Astronomicae. Anni...Ad Meridianum Mediolanensem
Informazioni su questo libro Si tratta della copia digitale di un libro che per generazioni è stato conservata negli scaffali di una biblioteca prima di essere digitalizzato da Google nell’ambito del progetto volto a rendere disponibili online i libri di tutto il mondo. Ha sopravvissuto abbastanza per non essere più protetto dai diritti di copyright e diventare di pubblico dominio. Un libro di pubblico dominio è un libro che non è mai stato protetto dal copyright o i cui termini legali di copyright sono scaduti. La classificazione di un libro come di pubblico dominio può variare da paese a paese. I libri di pubblico dominio sono l’anello di congiunzione con il passato, rappresentano un patrimonio storico, culturale e di conoscenza spesso difficile da scoprire. Commenti, note e altre annotazioni a margine presenti nel volume originale compariranno in questo file, come testimonianza del lungo viaggio percorso dal libro, dall’editore originale alla biblioteca, per giungere fino a te. Linee guide per l’utilizzo Google è orgoglioso di essere il partner delle biblioteche per digitalizzare i materiali di pubblico dominio e renderli universalmente disponibili. I libri di pubblico dominio appartengono al pubblico e noi ne siamo solamente i custodi. Tuttavia questo lavoro è oneroso, pertanto, per poter continuare ad offrire questo servizio abbiamo preso alcune iniziative per impedire l’utilizzo illecito da parte di soggetti commerciali, compresa l’imposizione di restrizioni sull’invio di query automatizzate. Inoltre ti chiediamo di: + Non fare un uso commerciale di questi file Abbiamo concepito Google Ricerca Libri per l’uso da parte dei singoli utenti privati e ti chiediamo di utilizzare questi file per uso personale e non a fini commerciali.
[Show full text]
Liste Des Juges
Liste des juges Jean-François VANAKEN (Belgique) Norman DESCHUYMERE (Belgique) Walter VAN DEN BROECK (Belgique) Elisabeth FEUZ (Suisse) Aida RIVERA (Colombie) Juan A. GRILLO (Colombie) Horst KLIEBENSTEIN (Allemagne) Istvan CSIK (Allemagne) Siret LEPASAAR (Estonie) Jean-Jacques MORBELLI (France) Jussi LIIMATAINEN (Finlande) Frank KANE (Royaume-Uni) Roger CROOKS (Royaume-Uni) Ildiko MUZSLAI (Hongrie) Manola POGGESI (Italie) Massimo INZOLI (Italie) Sonia FALLETTI-BELLAN (Italie) Andi HUDONO (Indonésie) Yolanda NAGLER-MAGAL (Israël) Michael LEONARD (Irlande) Gloria WAGNER (Luxembourg) Laurent HEINESCHE (Luxembourg) Ruth WAGNER (Luxembourg) Oystein EIKESETH (Norvège) Wenche EIKESETH (Norvège) Gerard JIPPING (Pays-Bas) John WILLIAMS (Pays-Bas) Zeferino Jose Cardoso SILVA (Portugal) Jan GAJEWSKI (Pologne) Malgorzata HALAS (Pologne) Blaz KAVCIC (Slovénie) Marija KAVCIC (Slovénie) Tatjana UREK (Slovénie) Bratislav MILOSEVIC (Serbie) Ozan BELKIS (Turquie) Donavon THOMPSON (Etats Unis d'Amérique) 90th International Dog Show - Chiens exposés par pays. Pays Nombre Country France 1726 France Allemagne 1102 Deutschland Belgique 857 België Pays-Bas 543 Nederland Espagne 150 España Italie 141 Italia Luxembourg 125 Lëtzebuerg Danemark 100 Danmark Suisse 93 Schweiz Royaume-Uni 87 Great Britain Russie 74 Rossijskaja Federazija République tchèque 60 Ceskà republika Pologne 44 Polska Hongrie 27 Magyarország Ukraine 25 Ykpaïha Irlande 22 Éire Roumanie 15 România Autriche 14 Österreich Suède 13 Sverige Portugal 10 Portugal Norvège 8 Norge Slovénie 8 Slovenija Croatie 8 Hrvatska Lettonie 7 Latvija Serbie 4 Srbija Finlande 4 Suomi Bulgarie 3 Balgarija Slovaquie 3 Slovensko Etats Unis d'Amérique 2 United States of America Estonie 2 Eesti Grèce 2 Elláda Montenegro 1 Crna Gora Lituanie 1 Lietuva Total 5281 Total Race/Breed Ring Chiens/Dogs Groupe F.C.I.
[Show full text]
Binary Star Studies with NPOI
CHARA/NPOI 2013 Science & Technology Review Binary studies with the Navy Precision Optical Interferometer Christian Hummel (ESO) Robert Zavala (USNO), Jason Sanborn (NAU, Lowell) + collaborators CHARA/NPOI 2013 Science & Technology Review Some current projects • Zeta Orionis – 7 year orbit, only recently finished after discovery in 2000 • Sigma Orionis – NPOI’s most “frustrating” target • Xi Tauri – Unknown origin, then “revived” by Petr Harmanec • HR 6493 – Forgotten, then “revived” by Shulin Ren • b Per • delta Lib CHARA/NPOI 2013 Science & Technology Review ζ Ori σ Ori CHARA/NPOI 2013 Science & Technology Review Zeta Orionis Ab B0.5V O9.5I (V=2.0) 40 mas Discovered by Hummel et al. 2000, predicted by Hanbury Brown et al. 1974 CHARA/NPOI 2013 Science & Technology Review The orbit after 7 years CHARA/NPOI 2013 Science & Technology Review Spectroscopy and radial velocities CHARA/NPOI 2013 Science & Technology Review Radial velocity fitting CHARA/NPOI 2013 Science & Technology Review System parameters CHARA/NPOI 2013 Science & Technology Review Evolutionary status of Zeta Orionis Aa+Ab CHARA/NPOI 2013 Science & Technology Review Sigma Orionis • AB = O9.5V + early BV, P = 157 yrs • Member of Sigma Ori cluster • Aa – Ab: 143 days • Ab: B0.5 V Simon-Diaz et al. 2011 Turner et al. 2008 CHARA/NPOI 2013 Science & Technology Review Tertiary component detected by NPOI Data from March 25, 2010 Turner et al. 2008 prediction Fit with improved orbit CHARA/NPOI 2013 Science & Technology Review Modifying Turner’s 2008 orbit CHARA/NPOI 2013 Science & Technology Review Sigma Orionis: close-pair orbit • a = 4.3 mas • e = 0.784 Peterson (priv.
[Show full text]
Sternenhimmel
Sternenhimmel Daniela Huber Ebenböckstraße 10 81241 München 089/97392937, Deutschland [email protected] Abstract In dem Projekt „Sternenhimmel“ geht es darum, sich die 12 Tierkreiszeichen der Sternbilder einzeln anzuschauen. Die Sterne werden durch LEDs verkörpert, die an einem schwarzen Regenschirm angebracht wurden. Über eine Eingabe am Laptop und die Verarbeitung der Eingabe mittels eines Arduino Mega, ist es möglich, zwischen den einzelnen Sternbildern zu wechseln und auch Informationen zu jedem Stern zu erhalten. Categories and Subject Descriptors • Human-centered computing~Information visualization General Terms Design, Experimentieren und Performance. Keywords „Innovativer Regenschirm“ – „Sternenkunde unter dem Regenschirm“ 1. Motivation Das Thema hat mich sehr interessiert, da ich mir ein Projekt mit LEDs vorgestellt hatte, die man in irgendeiner Weise über das Arduino Mega steuern kann. Eine gute Gelegenheit hierfür bietet die Darstellung von Sternenhimmeln, wie es auch schon in verschiedenen Einrichtungen wie z.B. Schwimmbädern oder Museen der Fall ist. 2. Verwandte Arbeiten Bei den verwandten Arbeiten sind LED-Sternenhimmel zu nennen, die man kaufen kann, um sie in der Wohnung an der Decke anzubringen. Außerdem verwandt zu meinem Thema sind die LED-Sternenhimmel in verschiedenen Schwimmbädern beispielsweise über Ruhebecken, um sich zu entspannen. Auch für den Innenbereich eines Autos gibt es schon Sternenhimmel aus LEDs zum Anbringen. Eine sehr eng verwandte Arbeit ist der Regenschirm mit eingezeichneten Sternbildern, welcher jedoch keine LEDs beinhaltet. Quelle: unterwegs-magazin.de Quelle: planetarium-hamburg.de Des Weiteren gibt es auch schon Schirme mit integrierten Lichtern, bei denen hingegen keine Sternbilder aufgezeigt, oder sogar ausgewählt werden können. Meine Arbeit verbindet nun die beiden genannten Regenschirmbeispiele und fügt noch die Funktionen hinzu, zwischen den einzelnen Sternbildern zu wechseln und sich Informationen zu den einzelnen Sternen anzeigen zu lassen.
[Show full text]
The X-Ray Puzzle of the L1551 IRS 5 Jet
A&A 530, A123 (2011) Astronomy DOI: 10.1051/0004-6361/201016305 & c ESO 2011 Astrophysics The X-ray puzzle of the L1551 IRS 5 jet P. C. Schneider1, H. M. Günther2, and J. H. M. M. Schmitt1 1 Hamburger Sternwarte, Gojenbergsweg 112, 21029 Hamburg, Germany e-mail: [cschneider;jschmitt]@hs.uni-hamburg.de 2 Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA, USA e-mail: [email protected] Received 13 December 2010 / Accepted 18 April 2011 ABSTRACT Protostars are actively accreting matter and they drive spectacular, dynamic outflows, which evolve on timescales of years. X-ray emission from these jets has been detected only in a few cases and little is known about its time evolution. We present a new Chandra observation of L1551 IRS 5’s jet in the context of all available X-ray data of this object. Specifically, we perform a spatially resolved spectral analysis of the X-ray emission and find that (a) the total X-ray luminosity is constant over almost one decade, (b) the majority of the X-rays appear to be always located close to the driving source, (c) there is a clear trend in the photon energy as a function of the distance to the driving source indicating that the plasma is cooler at larger distances and (d) the X-ray emission is located in a small volume which is unresolved perpendicular to the jet axis by Chandra. A comparison of our X-ray data of the L1551 IRS 5 jet both with models as well as X-ray observations of other protostellar jets shows that a base/standing shock is a likely and plausible explanation for the apparent constancy of the observed X-ray emission.
[Show full text]
Low Mass Star Formation in the Taurus-Auriga Clouds
Handbook of Star Forming Regions Vol. I Astronomical Society of the Paciﬁc, 2008 Bo Reipurth, ed. Low Mass Star Formation in the Taurus-Auriga Clouds Scott J. Kenyon Smithsonian Astrophysical Observatory, 60 Garden Street Cambridge, MA 02138, USA Mercedes Gomez´ Observatorio Astronomico,´ Universidad Nacional de Cor´ doba Laprida 854, 5000 Cor´ doba, Argentina Barbara A. Whitney Space Science Institute, 4750 Walnut Street, Suite 205 Boulder, CO 80301, USA Abstract. We review the history and structure of star formation in the Taurus-Auriga dark clouds. Our discussion includes a summary of the macroscopic cloud properties, the population of single and binary pre-main sequence stars, the properties of jets and outﬂows, and detailed summaries of selected individual objects. We include compre- hensive tables of dark clouds, young stars, and jets in the clouds. 1. Overview In October 1852, J. R. Hind `noticed a very small nebulous looking object' roughly 1800 west of a tenth magnitude star in Taurus. Over the next 15 years, the nebula slowly faded in brightness and in 1868 vanished completely from the view of the largest tele- scopes. O. Struve then found a new, smaller and fainter, nebulosity roughly 40 west of Hind's nebula. While trying to recover these nebulae, Burnham (1890, 1894) discov- ered a small elliptical nebula surrounding T Tau (Figure 1). Spectra of Hind's nebula revealed emission from either Hβ or [O III] λ5007, demonstrating that the nebula was gaseous as in novae and planetary nebulae. At about the same time, Knott (1891) reported 4 magnitude variability in the `ruddy' star associated with these nebulae, T Tauri.
[Show full text]
Snake River Skies the Newsletter of the Magic Valley Astronomical Society
Snake River Skies The Newsletter of the Magic Valley Astronomical Society December 2020 MVAS President’s Message Membership Meeting See President’s Message for December Centennial Observatory Due to the need to maintain social Colleagues, distance during the Covid-19 pandemic, access to the observatory It is argued that one cannot fight the weather. However, we have learned that we dome is one small group at a time. st can adapt and deal with it. The weather was indeed a challenge to the Dec. 21 Faulkner Planetarium Jupiter-Saturn conjunction. I was at the Herrett Center with Chris Anderson that See inside for Details day, and the two planets stayed behind the clouds until the very last moment. Even www.mvastro.org in that case, I was unable to image the two because the battery on my laptop went out. However, because the two still stayed close, I was able to do some imaging Club Officers the next day, but again the wind and clouds weakened the images. Robert Mayer, President Not only does astronomy give us the opportunity to learn to adapt, but it also [email protected] requires us to take a longer perspective. Too often, I get wrapped up with what dim planetary nebula a high-power eyepiece in a large aperture telescope can look like Gary Leavitt, Vice President at that moment, but I often forget that astronomy is just as pleasurable at wider [email protected] fields of view over longer periods of time. Stepping outside in the evening to watch the two planets come together and then separate over the past four five weeks has Dr.
[Show full text]
The COLOUR of CREATION Observing and Astrophotography Targets “At a Glance” Guide
The COLOUR of CREATION observing and astrophotography targets “at a glance” guide. (Naked eye, binoculars, small and “monster” scopes) Dear fellow amateur astronomer. Please note - this is a work in progress – compiled from several sources - and undoubtedly WILL contain inaccuracies. It would therefor be HIGHLY appreciated if readers would be so kind as to forward ANY corrections and/ or additions (as the document is still obviously incomplete) to: [email protected]. The document will be updated/ revised/ expanded* on a regular basis, replacing the existing document on the ASSA Pretoria website, as well as on the website: coloursofcreation.co.za . This is by no means intended to be a complete nor an exhaustive listing, but rather an “at a glance guide” (2nd column), that will hopefully assist in choosing or eliminating certain objects in a specific constellation for further research, to determine suitability for observation or astrophotography. There is NO copy right - download at will. Warm regards. JohanM. *Edition 1: June 2016 (“Pre-Karoo Star Party version”). “To me, one of the wonders and lures of astronomy is observing a galaxy… realizing you are detecting ancient photons, emitted by billions of stars, reduced to a magnitude below naked eye detection…lying at a distance beyond comprehension...” ASSA 100. (Auke Slotegraaf). Messier objects. Apparent size: degrees, arc minutes, arc seconds. Interesting info. AKA’s. Emphasis, correction. Coordinates, location. Stars, star groups, etc. Variable stars. Double stars. (Only a small number included. “Colourful Ds. descriptions” taken from the book by Sissy Haas). Carbon star. C Asterisma. (Including many “Streicher” objects, taken from Asterism.
[Show full text]
LESSON 1A: WELCOME and INTRODUCTIONS
LESSON 1a: WELCOME AND INTRODUCTIONS What you will need: • RASC membership application forms. • Stick on nametag labels and a black felt marker to write on them. • Binders for each student to put their lesson handouts in. • Course overview with the date and time of each lesson for each student Suggested Outline: • Collect money and membership information from any who have not already registered. • Have students put on nametags. • Have students introduce themselves and tell why they chose to take the course. • Hand out course overview and binder for students to put their handouts in throughout the course. • Explain that the cost of the course included one-year membership in the RASC your Centre and the Beginner’s Observing Guide. • Show and discuss the RASC publications. • Tour the observatory. LESSON 1b: OBSERVING What you will need: • A copy of the Beginner’s Observing Guide for each student • Explore the Universe Program Guideline for each student • A copy of Skyways for the teacher • A copy of the handouts for each student. Suggested Outline: • Hand out & discuss Beginner’s Observing Guide and the Explore the Universe Certificate Program Guidelines (ETUC). • Hand out Preparing for an Observing Session article. • Discuss basic equipment: i.e. Red light, maps, clothing. (show observer’s bag) • Hand out The Observing Logbook article • Hand out RASC Visual Observing Log sheet (from RASC national website.) • Describe how to record observations using the sample observation form • Hand out & discuss Lunar Sketching for Fun article. • DEMO: have students observe file “#1 - Observing Slides” on a data projector (or use overheads provided) and fill out a RASC Visual Observing Log sheet.
[Show full text]